Chapter 3 Acceleration and free fall - Light and Matter
Chapter 3 Acceleration and free fall - Light and Matter
Chapter 3 Acceleration and free fall - Light and Matter
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Summary<br />
Selected vocabulary<br />
gravity . . . . . . A general term for the phenomenon of attraction<br />
between things having mass. The attraction<br />
between our planet <strong>and</strong> a human-sized object<br />
causes the object to <strong>fall</strong>.<br />
acceleration . . . The rate of change of velocity; the slope of the<br />
tangent line on a v − t graph.<br />
Notation<br />
vo . . . . . . . . . initial velocity<br />
vf . . . . . . . . . final velocity<br />
a . . . . . . . . . . acceleration<br />
g . . . . . . . . . . the acceleration of objects in <strong>free</strong> <strong>fall</strong>; the<br />
strength of the local gravitational field<br />
Summary<br />
114 <strong>Chapter</strong> 3 <strong>Acceleration</strong> <strong>and</strong> <strong>free</strong> <strong>fall</strong><br />
Galileo showed that when air resistance is negligible all <strong>fall</strong>ing<br />
bodies have the same motion regardless of mass. Moreover, their<br />
v − t graphs are straight lines. We therefore define a quantity called<br />
acceleration as the derivative dv/dt. This definition has the advantage<br />
that a force with a given sign, representing its direction, always<br />
produces an acceleration with the same sign. The acceleration of objects<br />
in <strong>free</strong> <strong>fall</strong> varies slightly across the surface of the earth, <strong>and</strong><br />
greatly on other planets.<br />
For motion with constant acceleration, the following three equations<br />
hold:<br />
∆x = vo∆t + 1<br />
2 a∆t2<br />
v 2 f = v2 o + 2a∆x<br />
a = ∆v<br />
∆t<br />
They are not valid if the acceleration is changing.